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(1 - 8 of 8)
KiDS-1000: combined halo-model cosmology constraints from galaxy abundance, galaxy clustering, and galaxy-galaxy lensing
KiDS-1000 cosmology: Constraints from density split statistics
KiDS-1000: Cosmology with improved cosmic shear measurements
Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction
Euclid preparation
KiDS and Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
Why are we still using 3D masses for cluster cosmology?
Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses